Epsilon Reticuli
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Epsilon Reticuli (ε Ret / ε Reticuli) is a 4th magnitude star in the constellation Reticulum. The system is a binary, the primary component being an orange subgiant, and the secondary is probably a red dwarf. The primary star should be easily visible without optical aid under dark skies in southern hemisphere.
The primary star is known to have an extrasolar planet orbiting it.
ε Reticuli A
The primary star, ε Reticuli A, is a yellow subgiant 20% more massive than our Sun. Being a subgiant it is ceasing or has already ceased fusing hydrogen in its core. Soon the star will swell up and become a red giant. Despite its advanced stage, it cannot be much older than the Sun.
ε Reticuli Ab
The planet, designated as ε Reticuli Ab, was discovered in 2001 by the Anglo-Australian Planet Search Team using the highly successful radial velocity method. The planet is at least 28% more massive than Jupiter, but as the inclination of the planet's orbit is not known, it may be more massive.
The planet orbits the star in a very Earth-like orbit. However, the planet is certainly a gas giant and life as we know it may not flourish there. The planet may have massive moons (they cannot be detected with current technology) that could have supported life, but as the star aged they became too hot for life.
ε Reticuli B
The companion star, ε Reticuli B is likely a dim red dwarf. Not much information is available on it.
References
External links
- [SIMBAD] [component A entry], [component B entry], [planet entry]
- [The Extrasolar Planets Encyclopaedia] [entry]
- [ε Reticuli] at Extrasolar Visions
- [ε Reticuli Ab] at Extrasolar Visions
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